The Parkes Multibeam Pulsar Survey: I. Observing and Data Analysis Systems, Discovery and Timing of 100 Pulsars

Abstract

The Parkes multibeam pulsar survey is a sensitive survey of a strip along the Galactic plane with |b|<5 deg and l=260 deg to l=50 deg. It uses a 13-beam receiver on the 64-m Parkes radio telescope, receiving two polarisations per beam over a 288 MHz bandwidth centred on 1374 MHz. Receiver and data acquisition systems are described in some detail. For pulsar periods in the range 0.1 - 2 s and dispersion measures of less than 300 cm^{-3} pc, the nominal limiting flux density of the survey is about 0.2 mJy. At shorter or longer periods or higher dispersions, the sensitivity is reduced. Timing observations are carried out for pulsars discovered in the survey for 12 - 18 months after confirmation to obtain accurate positions, spin parameters, dispersion measures, pulse shapes and mean flux densities. The survey is proving to be extremely successful, with more than 600 pulsars discovered so far. We expect that, when complete, this one survey will come close to finding as many pulsars as all previous pulsar surveys put together. The newly discovered pulsars tend to be young, distant and of high radio luminosity. They will form a valuable sample for studies of pulsar emission properties, the Galactic distribution and evolution of pulsars, and as probes of interstellar medium properties. This paper reports the timing and pulse shape parameters for the first 100 pulsars timed at Parkes, including three pulsars with periods of less than 100 ms which are members of binary systems. These results are briefly compared with the parameters of the previously known population.

35 pages, 7 figures, 7 tables. Accepted by MNRAS

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• Detections of millisecond pulsars with the Fermi Large Area Telescope
• Young neutron stars with soft gamma ray emission and anomalous X-ray pulsar
• SPARKESX: Single-dish PARKES data sets for finding the uneXpected -- A data challenge
• An Arecibo Search for Fast Radio Transients from M87
• Pulsar discovery prospect of FASTA
• Evidence for the spin-kick alignment of pulsars from the statistics of their magnetic inclinations
• Multifrequency Strategies for the Identification of Gamma-Ray Sources
• Radio pulsar population synthesis with consistent flux measurements using simulation-based inference
• Harmonic Summing Improves Pulsar Detection Sensitivity: A Probability Analysis
• TRAPUM pulsar and transient search in the Sextans A and B galaxies and discovery of background FRB 20210924D
• Are the infrared-faint radio sources pulsars?
• Magnetic braking of Ap/Bp stars: an alternative formation mechanism of compact intermediate-mass binary pulsars
• Possible counterpart signal of the Fermi bubbles at the cosmic-ray positrons
• A multifrequency characterization of the extragalactic hard X-ray sky
• Pulsar Population Synthesis with Magnetorotational Evolution: Constraining the Decay of Magnetic field
• Dealing with the data imbalance problem on pulsar candidates sifting based on feature selection
• Pulsars as Fantastic Objects and Probes
• A study of dynamical effects in the observed second time-derivative of the spin or orbital frequencies of pulsars
• Installation and Use of Pulsar Search Software
• A Method for Pulsar Searching: Combining a Two-dimensional Autocorrelation Profile Map and a Deep Convolutional Neural Network
• The High Time Resolution Universe surveys for pulsars and fast transients
• Triple trouble with PSR J1618-3921: Mass measurements and orbital dynamics of an eccentric millisecond pulsar
• Transient Radio Neutron Stars
• Deep Synoptic Array Science: Searching for Long Duration Radio Transients with the DSA-110
• Application of Efron-Petrosian method to radio pulsar fluxes
• Big Data Challenges of FAST
• Timing observations of three Galactic millisecond pulsars
• The Galactic population of canonical pulsars
• Pulsar Observations with the Fermi Large Area Telescope
• 4-8 GHz Fourier-domain Searches for Galactic Center Pulsars
• High Energy Radiation from Spider Pulsars
• Constraining the selection corrected luminosity function and total pulse count for radio transients
• A magnetospheric dichotomy for pulsars with extreme inclinations
• PSR J2021+3651: A New Gamma-Ray Pulsar Candidate
• Discovery of the candidate pulsar wind nebula HESS J1718-385 in very-high-energy gamma-rays